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150

Zitterbewegung (Trembling Motion) of in

Tomasz M. Rusin1 and Wlodek Zawadzki2 1Orange Customer Service sp. z o. o., Warsaw 2Institute of , Polish Academy of Sciences, Al. Lotników, Warsaw Poland

1. Introduction This chapter describes a somewhat mysterious phenomenon known in the literature under the German name of “Zitterbewegung” (trembling motion). Both the phenomenon and its name were conceived by Erwin Schrodinger who, in 1930, published the paper Ueber die kraeftefreie Bewegung in der relativistischen Quantenmechanik in which he observed that in the , describing relativistic electrons in a vacuum, the 4 4 operators corresponding to × components of relativistic velocity do not commute with the free- Hamiltonian (Barut & Bracken, 1981; Schroedinger, 1930). In consequence, the electron velocity is not a constant of the motion also in absence of external fields. Such an effect in a vacuum must be of a quantum as it does not obey Newton’s first law of classical motion. Schrodinger calculated the resulting time dependence of the electron velocity and position concluding that, in addition to classical motion, they experience very fast periodic oscillations which he called Zitterbewegung (ZB). Schrodinger’s idea stimulated numerous theoretical investigations but no experiments since the predicted frequencyh ¯ ω 2m c2 1 MeV and the amplitude Z ≃ 0 ≃ of about λ = h¯ /mc 3.86 10 3Å are not accessible to current experimental techniques. It c ≃ × − was recognized that the ZB is due to an interference of states corresponding to the positive and negative electron energies resulting from the Dirac equation (Bjorken & Drell, 1964; Greiner, 1994; Sakurai, 1997). Lock (1979) showed that, if an electron is represented by a wave packet, its ZB has a transient character, i.e. it disappears with time. It was conceived years later that the trembling electron motion should occur also in crystalline solids if their band structure could be represented by a two-band model reminiscent of the Dirac equation (Cannata et al., 1990; Lurie & Cremer, 1970; Vonsovskii et al., 1990; Zawadzki, 1997). An intense interest in ZB of electrons in semiconductors was launched only in 2005 (Schliemann et al., 2005; Zawadzki, 2005). There followed a wave of theoretical considerations for various semiconductor and other systems. It was recognized that the phenomenon of ZB occurs every time one deals with two or more interacting energy bands (Cserti & David, 2006; Rusin & Zawadzki, 2007a; Winkler et al., 2007). As mentioned above, in a vacuum the ZB characteristics are not favorable. In solids, the ZB characteristics are much better but it is difficult to observe the motion of a single electron. However, recently Gerritsma et al. (2010) simulated experimentally the Dirac equation and

www.intechopen.com 2294 GrapheneWill-be-set-by-IN-TECH Simulation the resulting electron Zitterbewegung with the use of trapped ions and laser excitations. The power of the simulation method is that one can adjust experimentally the essential parameters of the Dirac equation: mc2 and c, and thus achieve more favorable values of the ZB frequency and amplitude. Interestingly, it turned out that analogues of ZB can occur also in classical wave propagation phenomena. Several predictions were made, but in two systems, namely macroscopic sonic crystals (Zhang & Liu, 2008), and photonic superlattices (Dreisow et al., 2010), the ZB-like effects were actually observed.

2. ZB of electrons in graphene Here we consider the ZB in three modern materials: monolayer graphene, bilayer graphene and carbon nanotubes. Monolayer graphene is currently by far the most studied material in the world (Novoselov et al., 2004). The description is based mostly on our theoretical works (Rusin & Zawadzki, 2007b; 2008; 2009), but papers of other authors concerned with ZB in graphene are also mentioned. It is emphasized that the trembling electrons should emit electromagnetic radiation which would provide a direct evidence for the existence of this phenomenon. We discuss the origin of ZB in crystalline solids not going into detailed mathematical derivations. An exact formulation of the electron dynamics in monolayer graphene in the presence of a magnetic field is presented in Appendix A. The electron classical velocity and its mass for a linear energy band of monolayer graphene are considered in Appendix B. It is hoped that our presentation will simulate experimental investigations of the electron trembling motion in graphene.

2.1 Bilayer graphene We begin our description considering bilayer graphene since the results can be obtained in the analytical form, which allows one to see directly important features of the trembling motion. Two-dimensional Hamiltonian for bilayer graphene in the K point of Brillouin zone is (McCann & Fal’ko, 2006)

1 0 (pˆ ipˆ )2 Hˆ = x − y , (1) B − 2m (pˆ + ipˆ )2 0 ∗  x y  where m = 0.054m . The energy spectrum is = E , where E = h¯ 2k2/2m , i.e. there is ∗ 0 Ek ± k k ∗ no energy gap between the parabolic conduction and valence bands. The position operator in the is a 2 2 matrix xˆ(t)=exp(iHˆ t/¯h)xˆ exp( iHˆ t/¯h). One calculates × B − B 2 ky hk¯ t x (t)=x(0)+ 1 cos , (2) 11 k2 − m   ∗  2 2 2 where k = kx + ky. The third term represents the Zitterbewegung with the frequency 2 2 h¯ ωZ = 2¯h k /2m∗, corresponding to the energy difference between the upper and lower energy branches for a given value of k. We want to calculate the ZB of a charge carrier represented by a two-dimensional wave packet

1 d 2 1 d2k2 1 d2(k k )2 ikr 1 ψ(r,0)= d ke− 2 x − 2 y− 0y e . (3) 2π √π 0   

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The packet is centered at k0 =(0, k0y) and is characterized by a width d. The unit vector (1, 0) is a convenient choice, selecting the (11) component of xˆ(t), see Eq. (2). An average of xˆ11(t) is a two-dimensional integral which can be calculated analytically in the form

x¯ (t)= ψ(r) xˆ(t) ψ(r) = x¯ + x¯ (t) (4) 11  | |  c Z where x¯ =(1/k ) 1 exp( d2k2 ) , and c 0y − − 0y   4 2 2 2 4 2 1 δ d k δ d k ( )= 0y 0y x¯Z t exp 4 4 cos 4 4 k0y − d + δ d + δ exp( d2k2 ) , (5) − − 0y  in which δ = √ht¯ /m∗ contains the time dependence. In Figure 1a we show the ZB of the electron position x¯11 as given in Eqs. (4) and (5). Here are the main features of ZB following from Eqs. (4) and (5). First, in order to have ZB in the direction x one needs an initial transverse momentumhk ¯ 0y. Second, the ZB 2 4 4 4 frequency depends only weakly on the packet width: ωZ =(hk¯ 0y/m∗)(d /(d + δ )), while its amplitude is strongly dependent on the width d. Third, the ZB has a transient character since it is attenuated by the exponential term. For small t the amplitude of x¯Z(t) diminishes as exp( Γ2 t2) with − Z hk¯ 0y ΓZ = . (6) m∗d Fourth, as t (or δ) increases, the cosine term tends to unity and the first term in Eq. (5) cancels out with the second term. After the oscillations disappear, the charge carrier is displaced by the amount x¯c, which is a “remnant” of ZB. Fifth, for very wide packets (d ∞) the exponent 2 2 → in Eq. (5) tends to unity, the oscillatory term is cos(δ k0y) and the last term vanishes. In this limit one recovers undamped ZB oscillations. Next, we consider other quantities related to ZB, beginning by the current. The latter is given by the velocity multiplied by charge. The velocity is simply v¯x = ∂x¯Z/∂t, where x¯Z is given by Eq. (5). The calculated current is plotted in Figure 1b, its oscillations are a direct manifestation of ZB. The transient character of ZB is accompanied by a temporal spreading of the wave packet. The question arises whether the attenuation of ZB is not simply caused by the spreading of the packet. The calculated packet width ΔR is plotted versus time in Figure 1c. It is seen that during the initial 80 femtoseconds the packet’s width increases only twice compared to its initial value, while the ZB disappears almost completely. We conclude that the spreading of the packet is not the main cause of the transient character of ZB. Looking for physical reasons behind the transient character of ZB we decompose the total ψ(r, t) into the positive (p) and negative (n) components ψp(r, t) and ψn(r, t). We have

ˆ ψ(t) = e iHt/¯h ψ(0) |  − |  = e iEt/¯h p ψ(0) p + eiEt/¯h n ψ(0) n , (7) −  | |   | | 

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40

20 x(t) x(t) (A) a 0 0.10

0.05 jx(t) 0.00 -0.05 (t) (pAm) x j -0.10 b

600 500 c

R(t) (A) 400 ΔR(t) Δ 300 200 0 1020304050607080t (fs) Fig. 1. Zitterbewegung of a charge carrier in bilayer graphene versus time, calculated for a gaussian wave packet width d = 300Å and k = 3.5 108m 1: a) position, b) electric 0y × − current, c) dispersion ΔR(t). After the ZB disappears a constant shift of the position remains. After Rusin & Zawadzki (2007b). where p and n are the eigen-functions of the Hamiltonian (1) in k space corresponding to |  |  positive and negative energies, respectively. Further

1 1 k p = δ(k k′ ), (8)  |  √ k2 /k2 − 2  +  1 1 k n = δ(k k′ ). (9)  |  √ k2 /k2 − 2  − +  After some manipulations we obtain

p 1 d 2 1 d2(k2 +(k k )2) ikr iEt/¯h ψ (r, t)= d ke− 2 x y − 0y e e− π 4 √π  × 1 . (10) k2 /k2  +  The function ψn(r, t) is given by the identical expression with the changed signs in front of E and k2 /k2 terms. There is ψ(r, t)=ψp(r, t)+ψn(r, t) and ψn ψp = 0. Now, one can +  |  calculate the average values of x¯ and y¯ using the positive and negative components in the above sense. We have x¯(t)= (ψn + ψp)†x(ψn + ψp)d2r, (11) 

www.intechopen.com Zitterbewegung (Trembling Motion) Zitterbewegungof Electrons in Graphene (Trembling Motion) of Electrons in Graphene 2975 so that one deals with four integrals. A direct calculation gives

p 2 2 n 2 2 ψ xd r + ψ xd r = x¯c, (12)  | |  | | n† p 2 p† n 2 ψ xψ d r + ψ xψ d r = x¯Z(t), (13)   where x¯c and x¯Z(t) have been defined in Eq. (4). Thus the integrals involving only the positive and only the negative components give the constant shift due to ZB, while the mixed terms lead to the ZB oscillations. All terms together reconstruct the result from Eq. (4). Next we calculate the average value y¯. There is no symmetry between x¯ and y¯ because the wave packet is centered around kx = 0 and ky = k0y. The average value y¯ is again given by four integrals. However, now the mixed terms vanish, while the integrals involving the positive and negative components give

hk¯ 0y ψp 2yd2r = t, (14) m  | | 2 ∗ hk¯ 0y ψn 2yd2r = t. (15) m  | | − 2 ∗ This means that the “positive” and “negative” subpackets move in the opposite directions rel with the velocity v = hk¯ 0yt/2m∗. The relative velocity is v = hk¯ 0yt/m∗. Each of these Γ 1 rel packets has the initial width d and it (slowly) spreads in time. After the time −Z = d/v the distance between the two packets equals d, so the integrals in Eq. (12) are small, resulting in the diminishing Zitterbewegung amplitude. This reasoning gives the decay constant ΓZ = hk¯ 0y/m∗d, which is exactly what we determined above from the analytical results (see Eq. (6)). Thus, the transient character of the ZB oscillations is due to the increasing spatial separation of the subpackets corresponding to the positive and negative energy states. This confirms our previous conclusion that it is not the packet’s slow spreading that is responsible for the attenuation. The separation of subpackets with the resulting decay of ZB turns out to be a general feature of this phenomenon.

2.2 Monolayer graphene Now we consider monolayer graphene. The two-dimensional band Hamiltonian describing its band structure at the K point of the Brillouin zone is (Semenoff, 1984; Slonczewski & Weiss, 1958; Wallace, 1947) 0 pˆ ipˆ Hˆ = u x − y , (16) M pˆ + ipˆ 0  x y  where u 1 108cm/s. The resulting energy dispersion is linear in momentum: = uhk¯ , ≈ × E ± 2 2 where k = kx + ky. The quantum velocity in the Schrodinger picture is vˆi = ∂HM/∂pˆi, it does not commute with the Hamiltonian (16). In the Heisenberg picture we havev ˆ(t)= exp(iHˆ t/¯h)vˆ exp( iHˆ t/¯h). Using Eq. (16) one obtains M − M ( ) ky v 11 = u sin(2ukt). (17) x k

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d= 10A 0.15 d= 20A d= 40A d= 80A 0.10 d=160A

0.05

0.00 (t) (pAm) x j -0.05

-0.10

-0.15

024681 t (fs)012 Fig. 2. Oscillatory electric current in the x direction caused by the ZB in monolayer graphene versus time, calculated for a gaussian wave packet with k = 1.2 109m 1 and various 0y × − packet widths d. Transient character of ZB is clearly seen. After Rusin & Zawadzki (2007b).

The above equation describes the trembling motion with the frequency ωZ = 2uk, determined by the energy difference between the upper and lower energy branches for a given value of k. As before, ZB in the direction x occurs only if there is a non-vanishing momentumhk ¯ y. One calculates an average velocity (or current) taken over a two-dimensional wave packet with nonzero initial momentum k0x. The results for the current j¯x = ev¯x are plotted in Figure 2 for different realistic packet widths d. It is seen that the ZB frequency does not depend on d and is nearly equal to ωZ given above for the plane wave. On the other hand, the amplitude of ZB depends on d and we deal with decay times of the order of femtoseconds. For small d there are almost no oscillations, for very large d the ZB oscillations are undamped. These conclusions agree with the analytical results for bilayer graphene. The behavior of ZB depends quite critically on the values of k0y and d, which is reminiscent of the damped harmonic oscillator. In the limit d ∞ the above results for the electric current resemble those of Katsnelson → (2006) for ZB in graphene obtained with the use of plane wave representation. Maksimova et al. (2008) investigated dynamics of wave packets in monolayer graphene for different pseudo- polarizations with the resulting ZB. For specific packet components and their relative phases a “longitudinal ZB” can take place, but its intensity is weak. Martinez et al. (2010) considered a creation of electron-hole pairs by a constant electric field in the plane of a monolayer graphene sheet. They showed that, as the pairs undergo the ZB in opposite directions, a Hall-like separation of the charge occurs giving a measurable dipole moment. We note that it is not the time-dependent motion but the ZB shift at large times which is responsible for the charge separation, see Eq. (2) and Figure 1. Englman &

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Vertesi (2008) calculated a ZB-related electron current in monolayer graphene in the adiabatic approximation and related it to the Berry phase.

2.3 Carbon nanotubes Finally we consider monolayer graphene sheets rolled into single semiconducting carbon nanotubes (CNT) (Rusin & Zawadzki, 2007b; Zawadzki, 2006). The band Hamiltonian in the vicinity of K point is (Ajiki & Ando, 1993)

0¯hk ipˆ Hˆ = u nν − y . (18) CNT hk¯ + ipˆ 0  nν y  This Hamiltonian is similar to that given by Eq. (16) except that, because of the periodic boundary conditions, the momentum px is quantized and takes discrete valueshk ¯ x = hk¯ nν, where k =(2π/L)(n ν/3), n = 0, 1,..., ν = 1, and L is the length of circumference nν − ± ± of CNT. As a result, the free electron motion can occur only in the direction y, parallel to the tube axis. The geometry of CNT has important consequences. There exists an energy gap E = 2uh¯ k and the effective mass at the band edge m = h¯ k /u. For ν = 1 there g | nν| 0∗ | nν| ± always exists a non-vanishing value of the quantized momentumhk ¯ nν. Finally, for each value of knν there exists k n, ν = knν resulting in the same subband energy = E, where − − − E ± 2 2 E = hu¯ knν + ky. (19)

The time dependent velocity vˆy(t) and the displacement yˆ(t) can be calculated for the plane electron wave in the usual way and they exhibit the ZB oscillations [see Zawadzki (2006)]. For small momenta k the ZB frequency ish ¯ ω = E and the ZB length is λ 1/ k .Weare y Z g Z ≈ | nν| again interested in the displacement y¯(t) of a charge carrier represented by a one-dimensional wave packet analogous to that described in Eq. (3) The average displacement is y¯(t)=y¯ (t) Z − y¯sh, where 2 2 ∞ h¯ du k dky 2Et 2 2 nν d ky y¯Z(t)= cos e− (20) 2√π ∞ E2 h¯ −   and y¯ = 1/2√πd sgn(b)[1 Φ( b )] exp(b2), where b = k d and Φ(x) is the error function. sh − | | nν The ZB oscillations of y¯(t) are plotted in Figure 3. It is seen that, after the transient ZB oscillations disappear, there remains a shift y¯sh. Thus the ZB separates spatially the charge carriers that are degenerate in energy but characterized by n, ν and n, ν quantum numbers. − − The current is proportional to v¯ = ∂y¯/∂t, so that the currents related to ν = 1 and ν = 1 y − cancel each other. To have a non-vanishing current one needs to break the above symmetry, which can be achieved by applying an external magnetic field parallel to the tube axis. It is seen from Figure 3 that the decay time of ZB in CNT is much larger than that in bilayer 1/2 and monolayer graphene. The oscillations decrease proportionally to t− . The reason is that we consider the situation with k0y = 0, so that the ZB oscillations occur due to “built in” momentum kx = knν, arising from the tube’s topology. In other words, the long decay time is due to the one-dimensionality of the system. If the circumference of a CNT is increased, the energy gap (and, correspondingly, the ZB frequency) decreases, the amplitude of ZB is larger, but the decay time remains almost unchanged. One can show that we again deal here with two sub-packets which, however, for k0y = 0 do not run away from each other. Thus, the slow damping of ZB is due only to the slow

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80 n=0 d=160A ν= 1 60

40 d=40A 20

0 y(t) (A) -20

-40

-60 n=0 -80 ν=-1

1 10 100t (fs) 1000 Fig. 3. Zitterbewegung of two charge carriers in the ground subband of a single carbon nanotube of L = 200 Å versus time (logarithmic scale), calculated for gaussian wave packets of two different widths d and k0y = 0. After the ZB disappears a constant shift remains. The two carriers are described by different quantum numbers ν. At higher times the amplitude of 1/2 ZB oscillations decays as t− . After Rusin & Zawadzki (2007b). broadening of the sub-packets. We emphasize the slow decay, as illustrated in Figure 3, because it is confirmed experimentally, see Gerritsma et al. (2010). We add that for k = 0 the 0y sub-packets run away from each other and the decay time is much faster.

3. ZB in graphene in a magnetic field The trembling motion of charge carriers in graphene and CNT has been described above for no external potentials. Now we consider the trembling motion of electrons in the presence of an external magnetic field (Rusin & Zawadzki, 2008). The magnetic field is known to cause no interband electron transitions, so the essential features of ZB are expected not to be destroyed. On the other hand, introduction of an external field provides an important parameter affecting the ZB behavior. This case is special because the electron spectrum is fully quantized, so we deal with discrete levels, not bands. We consider a graphene monolayer in an external magnetic field parallel to the z axis. The Hamiltonian for electrons and holes at the K1 point of the Brillouin zone is (Slonczewski & Weiss, 1958; Wallace, 1947)

0 πˆ iπˆ Hˆ = u x − y , (21) πˆ + iπˆ 0  x y 

www.intechopen.com Zitterbewegung (Trembling Motion) Zitterbewegungof Electrons in Graphene (Trembling Motion) of Electrons in Graphene 3019 where u 1 108 cm/s is the characteristic velocity,π ˆ = pˆ qAˆ is the generalized ≈ × − momentum, in which Aˆ is the vector potential and q is the electron charge. Using the Landau gauge, we take Aˆ =( By,0,0), and for an electron q = e with e > 0. We take the wave − − function in the form Ψ(x, y)=eikx xΦ(y). Introducing the magnetic radius L = √h¯ /eB, the variable ξ = y/L k L, and defining the standard raising and lowering operators for − x the harmonic oscillator aˆ =(ξ + ∂/∂ξ)/√2 and aˆ† =(ξ ∂/∂ξ)/√2, the Hamiltonian is − rewritten in the form 0 aˆ Hˆ = h¯ Ω , (22) − aˆ† 0   where the frequency is Ω = √2u/L. Next one determines the eigenstates and eigenenergies of the Hamiltonian Hˆ . The energy is E = sh¯ Ω√n. Here n = 0, 1, . . ., and s = 1 ns ± for the conduction and valence bands, respectively. The above energies were confirmed experimentally. The complete wave function is

eikx x s n 1 n nkxs = − | −  (23) | ≡|  √ n 4π  |   where n are the harmonic oscillator functions. |  We want to calculate the velocity of a charge carrier described by a wave packet. We first calculate matrix elements f n between an arbitrary two-component function f =(f u, f l)  |  and eigenstates from Eq. (23). A straightforward manipulation gives f n = sFu + Fl ,  |  − n 1 n where − j 1 j 1 ξ2 Fn(kx)= g (kx, y)e− 2 Hn(ξ)dy, (24) √2LCn  in which

j 1 j ikx x g (kx, y)= f (x, y)e dx. (25) √2π  The superscript j = u, l stands for the upper and lower components of the function f . The

Hamilton equations give the velocity components: vˆi(0)=∂Hˆ /∂pˆi, with i = x, y. We want to calculate averages of the time-dependent velocity operators vˆi(t) in the Heisenberg picture taken on the function f . The averages are

iE t/¯h iEnt/¯h v¯ (t)=∑ e n′ f n′ n′ v (0) n n f e− , (26) i  |  | i |  |  n,n′ where the energies and eigenstates are given in Eq. (23). The summation in Eq. (26) goes over all the quantum numbers: n, n′, s, s′, kx, k′x. The only non-vanishing matrix elements of the velocity components are for the states states n = n 1. One finally obtains ′ ±

dd d d cZ c  Z vtuVyn() œœ sin()XXXnn tuV sin()nn tiuA œ cos()nn tiuA œ cos() Xn t , (27) nn00 n  0 n  0

dd d d cZ c  Z vtuBxn() œœ cos()XXXXnn tuB cos(nn tiuT ) œœ sin()nn tiuT sin(n t ) , (28) nn00 n  0 n  0

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α,β where Vn±, Tn±, An± and Bn± are given by combinations of Um,n integrals

α,β α β Um,n = Fm∗(kx)Fn (kx)dkx. (29)  The superscripts α and β refer to the upper and lower components, see Rusin & Zawadzki α,β (2008). In the above model the coefficients Um,n are real numbers, so that An± and Tn± in Eqs. (27) and (28) vanish. The time dependent sine and cosine functions come from the c exponential terms in Eq. (26). The frequencies in Eqs. (27) and (28) are ωn = Ω(√n + 1 √n), Z c − ωn = Ω(√n + 1 + √n), where Ω is given in Eq. (22). The frequencies ωn correspond to the Z intraband energies while frequencies ωn correspond to the interband energies, see Figure 4. The interband frequencies are characteristic of the Zitterbewegung. The intraband (cyclotron) energies are due to the band quantization by the magnetic field and they do not appear for non quantized spectra. Final calculations are carried out for a two-dimensional Gaussian wave packet centered around the wave vector k0 =(k0x,0) and having two non-vanishing components. In this α,β case one can obtain analytical expressions for Um,n. The main frequency of oscillations is Ω c Ω Z Ω ω0 = , which can be interpreted either as ω0 = (√n + 1 √n) or ω0 = (√n + 1 + √n) c − Z for n = 0. Frequency ω0 belongs to the intraband (cyclotron) set, while ω0 belongs to the interband set (see Figure 4). The striking feature is, that ZB is manifested by several frequencies simultaneously. This is a consequence of the fact that in graphene the energy distances between c Z the Landau levels diminish with n, which results in different values of frequencies ωn and ωn for different n. It follows that it is the presence of an external quantizing magnetic field that introduces various frequencies into ZB. It turns out that, after the ZB oscillations seemingly die out, they actually reappear at higher times. Thus, for all k0x values (including k0x = 0), the ZB oscillations have a permanent character, that is they do not disappear in time. This feature is due to the discrete character of the electron spectrum caused by a magnetic field. The above property is in sharp contrast to the no-field cases considered above, in which the spectrum is not quantized and the ZB of a wave packet has a transient character. In mathematical terms, due to the discrete character of the spectrum, averages of operator quantities taken over a wave packet are sums and not integrals. The sums do not obey the Riemann-Lebesgues theorem for integrals which guarantee the damping of ZB in time for a continuous spectrum see Lock (1979). Finally, one calculates the displacements x¯(t) and y¯(t) of the wave packet. To this end we integrate Eqs. (27) and (28) with respect to time using the initial conditions x0 = x¯(0)=0 and y = y¯(0)=k L2. The results are plotted in Figure 5 in the form of x y trajectories for 0 x − different initial wave vectors k0x. The direction of movement is clockwise and the trajectories span early times (1ps) after the creation of a wave packet. All in all, the presence of a quantizing magnetic field has the following important effects on the trembling motion. (1) For B = 0 the ZB oscillation are permanent, while for B = 0 they are transient. The reason is that for B = 0 the electron spectrum is discrete. (2) For B = 0 many ZB frequencies appear, whereas for B = 0 only one ZB frequency exists. (3) For B = 0 both interband and intraband (cyclotron) frequencies appear in ZB; for B = 0 there are no intraband frequencies. (4) Magnetic field intensity changes not only the ZB frequencies but the entire character of ZB spectrum.

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n= 3 n= 2

E= -uhk n= 1 E= uhk

s= +1 k n=0 Energy

s= -1 hΩ

n= 1

n= 2

n= 3

Fig. 4. The energy dispersion E(k) and the Landau levels for monolayer graphene in a magnetic field (schematically). Intraband (cyclotron) and interband (ZB) energies for n = n 1 are indicated. The basic energy ish ¯ Ω = √2¯hu/L. After Rusin & Zawadzki ′ ± (2008).

The Zitterbewegung should be accompanied by electromagnetic dipole radiation emitted by the trembling electrons. The oscillations r(t) are related to the dipole moment e r(t) ,   −   which couples to the electromagnetic radiation. One can calculate the emitted electric field from the electron acceleration r¨(t ) and takes its Fourier transform to determine the emitted   frequencies. In Figure 6 we plot the calculated intensities of various emitted lines. The strong peak corresponds to oscillations with the basic frequency ω = Ω. The peaks on the high-frequency side correspond to the interband excitations and are characteristic of ZB. The peaks on the lower frequency side correspond to the intraband (cyclotron) excitations. In absence of ZB the emission spectrum would contain only the intraband (cyclotron) Z frequencies. Thus the interband frequencies ωn shown in Figure 6 are a direct signature Z of the trembling motion. It can be seen that the ωz peaks are not much weaker than the central peak at ω = Ω, which means that there exists a reasonable chance to observe them. Generally speaking, the excitation of the system is due to the nonzero momentumhk ¯ 0x given to the electron. It can be provided by accelerating the electron in the band or by exciting the electron with a nonzero momentum by light from the valence band to the conduction band. The electron can emit light because the Gaussian wave packet is not an eigenstate of the system described by the Hamiltonian (21). The energy of the emitted light is provided by the initial kinetic energy related to the momentumhk ¯ 0x. Once this energy is completely used, the emission will cease.

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-5 0x(t) (nm) 5 -5 0 5 x(t) (nm) 0 a b 0 y(t)-y (nm) 0 0 (nm) y(t)-y

-10 -20

0 c d 0 y(t)-y 0 (nm) (nm) 0 -40 y(t)-y

-40 -80 -10 0x(t) (nm) 10 -20 0x(t) (nm) 20

Fig. 5. Zitterbewegung trajectories of electron at the K1 point of the Brillouin zone in monolayer graphene at B=20T during the first picosecond for various values of k0x. After Rusin & Zawadzki (2008).

Schliemann (2008) described time dependence of the cyclotron motion in monolayer graphene in the presence of a magnetic field using the semiclassical approximation for high carrier energies. He showed that the cyclotron motion is perturbed by interband ZB contributions of higher frequencies. Krueckl & Kramer (2009) described time propagation of an initially concentrated wave packet in monolayer graphene in a perpendicular magnetic field. A collapse-revival pattern of ZB was investigated and an effect of impurities (disorder) on the packet dynamics was analyzed. It turned out that ZB “survives” the perturbation by impurities. Romera & de los Santos (2009) studied monolayer graphene in a magnetic field concentrating on collapse-revival pattern of ZB oscillations.

4. ZB probed by laser pulse All the recent theoretical work on ZB assumed that initially the electrons are represented by Gaussian wave packets. While this assumption represents a real progress compared to the work that had treated electrons as plane waves, it is obviously an idealization since it is not quite clear how to prepare an electron in this form. Here we calculate a reaction of an electron in graphene excited by a laser pulse, not assuming anything about initial form of the electron wave packet. In our description we take into account currently available experimental possibilities. The following conditions should be met for a successful observation of ZB: a) The ZB frequency must be in the range of currently detectable regimes, i.e. of the order of ω 1fs 1, Z ≈ −

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2.0 B=10T

1.5 Z ωc ω

Z ω 6 1.0 )(arb. units) )(arb. ω I( c ω Z 2 ω 0.5 c 1 ω 1

0.0 0.25 0.5 0.751 ω/Ω 2.5 5 7.5 Fig. 6. Intensity spectrum versus frequency during the first 20 ps of motion of an electron 1 described by a Gaussian wave packet having k0x = 0.035Å− in monolayer graphene. After Rusin & Zawadzki (2008). and the size of oscillations should be of the order of a few Å; b) The ZB oscillations should be persistent or slowly transient; c) Both positive and negative electron energies must be excited with a sufficient probability; d) The wave packet should be created in a one-electron regime. A system that fulfills the above criteria is p-type monolayer graphene in a constant magnetic field. The wave packet should be created by an ultra short monocycle or sub-monocycle laser pulse. Because of a very wide frequency spectrum of such a pulse, the resulting wave packet will have both positive and negative energies. The electron oscillations give rise to a time-dependent dipole moment which will be a source of electric field and it will emit or absorb radiation in the far infrared range. In the description we use the above results for the band structure of monolayer graphene in a magnetic field. The Fermi level is assumed to coincide with the Landau level (LL) n = 2 − and we consider the initial electron to be in the n = 1 state. The wavelength of the laser − light is assumed to be much larger that the size L of the n = 1 state, so we can neglect − spatial variation of the electric field in the laser pulse. The total Hamiltonian, including the perturbation due to the laser light, is Hˆ T = Hˆ + Wˆ (t), where Hˆ is given by Eq. (21) and the perturbing potential due laser light is

2 2 Wˆ (t)= ey e (2ln2)t /τ cos(ω t), (30) − E0 − L in which e is the electron charge, τ is the pulse duration (FWHM), ωL = 2πc/λL is the laser frequency (being of the order of 3 1015s 1), and is the amplitude of electric field. A × − E0

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Gaussian shape of the laser pulse is widely used in optical experiments and it parameterizes effectively a profile of electric field in the laser beam. iEk t/¯h As a result of a laser shot, the initial state of the system Φk(t)=ψke− evolves into iEjt/¯h ˆ the final state Ψk(t)=∑j cj(t)ψke− , which is a combination of the eigenstates of H with suitably chosen coefficients cj(t). The resulting time-dependent dipole moment is D(t)=e Ψk(t) r Ψk(t) . The corresponding time-dependent wave functions are Ψk(t)= iHtˆ /¯h  | |  e− Ψk(0), and the dipole moment is

ˆ ˆ D(t)=e Ψ (0)eiHt/¯h rˆ e iHt/¯hΨ (0)  k | | − k  = e Ψ (0) rˆ(t) Ψ (0) = e r(t) . (31)  k | | k    Here r(t) is the electron position in the Heisenberg picture. Thus the dipole moment D(t) is proportional to the time-dependent position averaged over the electron wave packet. A time-dependent dipole moment is a source of electromagnetic radiation. We treat the radiation classically (Bohm, 1952) and take the radiated transverse electric field to be (Jackson, 1975) D¨ (t) sin(θ) r ( , t)= 2 , (32) E⊥ 4πǫ0c R where ǫ0 is the vacuum permittivity, θ is an angle between the direction of electron motion and a position of the observer R. Since D¨ (t)=e r¨(t) , Eq. (32) relates the electric field of the   dipole with the average acceleration of the packet. If the electric field is measured directly by an antenna, one measures the trembling motion of the wave packet. If the square of electric field is measured in emission or absorption experiments, the signature of ZB is the existence of peaks corresponding to interband frequencies and their dependence on packet’s parameters. Accordingly, in the time resolved luminescence experiments it should be possible to detect directly the motion of the packet with interband frequencies. The electric field emitted by the trembling electron is calculated by the time-dependent perturbation theory. The induced dipole moment and the corresponding electric field oscillate with three frequencies. The frequency ω( 1 , 2+ )=(√2+ 1) Ω corresponds to the | − |  Zitterbewegung, i.e., to the motion of the packet with an interband frequency. Here 1 | − denotes the valence state n = 1 and 2+ the conduction state n = 2. The interband |  frequency is characteristic of ZB because the trembling motion occurs due to an interference of electron states related to positive and negative electron energies. The second frequency ω( 1 , 2 )=(√2 1) Ω describes the intraband cyclotron motion of the packet. The | − | − − third frequency ω( 1 , 0 )= Ω has both interband and intraband character (see Figure 4). | − |  In zero-gap materials like graphene the interband ZB frequency is not much larger than the cyclotron frequency. In Figure 7 we plot the oscillating dipole moment within the first 1000 fs of motion after the laser shot for two magnetic fields B = 1 T and B = 10 T, and two laser pulses. In Figure 8 we plot the corresponding electric field for the same parameters during the first 250 fs of oscillations. We assume the laser intensity to be I = 1.0 109 W/cm2, the emitted × electromagnetic wave detected at the angle θ = 45o, and the distance R = 1 cm. All the quantities in Figures 7 and 8 are calculated per one electron. Since the frequencies are incommensurable, the electron trajectories r(t) are not closed and there is no repeated pattern of oscillations. The motion of the wave packet is permanent in the time scale of femtoseconds

www.intechopen.com Zitterbewegung (Trembling Motion) Zitterbewegungof Electrons in Graphene (Trembling Motion) of Electrons in Graphene 30715 d y (t) 15(t) y 3 d 10 2

5 1

0 0

-5 -1 -10 a b -2 -15 -3

-15 -10 -5 0 5 10 15 dx-3(t) -2 -1 0 1 2 3 Fig. 7. Oscillations of dipole moment during the first 1000 fs of electron motion after the laser pulse. Experimental characteristics: pulse intensity 1 109 W/cm2,a)τ = 1.6 fs, B = 10 T, b) 28× τ = 3.0 fs, B = 10 T. Dipole moments in a) are in 10− [Cm] units, while in b) they are in 31 10− [Cm] units. The above results refer to very narrow Landau levels, disregarding broadening. After Rusin & Zawadzki (2009).

1.0 Ey

0.0 E (mV/m) -1.0 Ex b

Ey 5.0

V/m) 0.0 μ E ( -5.0

Ex d 0 50 100 150 200t (fs) 250 Fig. 8. Electric field emitted by one electron during the first 250 fs of electron motion after the laser pulse. Experimental characteristics: pulse intensity 1 109 W/cm2,a)τ = 1.6 fs, B = 10 × T, b) τ = 3.0 fs, B = 10 T. The above results refer to very narrow Landau levels, disregarding broadening. After Rusin & Zawadzki (2009). or picoseconds but there is damping of the motion due to the light emission in a long time scale. The results shown in Figures 7 and 8 refer to very narrow Landau levels, disregarding broadening. We can draw the following qualitative conclusions from Figure 7 and 8. First, for small magnetic fields B the period of oscillations is longer than for large fields, which is related to the basic frequency Ω. Second, irrespective of the variation of Ω with B, for small fields the oscillations are dominated by the low (cyclotron) frequency, while at stronger B the high (ZB) frequency dominates. Finally, comparing the magnitudes of dipole moment or emitted electric field for τ = 1.6 fs with the corresponding values for τ = 3.0 fs one observes that the amplitude of oscillations depends very strongly on the duration τ of the pulse.

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(0) E (0) E (0) x Ey x 1.0 (Γ) Ex 0.5

0.0 E (mV/m)

-0.5 (Γ) Ey -1.0

(0) Ey 0 100 200 300 t(fs)

Fig. 9. Calculated electric fields Ex(t) and Ey(t) emitted by one trembling electron during the first 400 fs after the laser pulse. Pulse parameters: intensity 1 109 W/cm2, τ = 1.6 fs, × magnetic field B = 1 T. Bold lines - electric fields for broadened Landau levels described by Lorentzian line-shapes with experimental values of Γn. Dotted lines - electric fields for delta-like Landau levels. After Rusin & Zawadzki (2009).

The broadening of the Landau levels may strongly influence the trembling motion of the wave packet. To analyze the overall impact of all the effects leading to the level broadening: disorder, e-e interaction, electron-phonon scattering, etc., one assumes finite widths of all energy levels, characterized by broadening parameters Γn. These are treated as phenomenological quantities determined experimentally and including all scattering mechanisms existing in real samples. We approximate the broadening of the density of states by a Lorentzian line-shape irrespective of the detailed scattering mechanism. The electric field E(t) is calculated, as before, as a second time derivative of D(t). In Figure 9 we plot the electric field emitted by an oscillating electron within the first 400 fs of motion after the laser shot of the width τ = 1.6 fs in a magnetic field B = 1 T. The two bold lines describe calculated electric fields Ex(t) and Ey(t) for the Landau levels having the broadening parameters Γn indicated above. The two dotted lines show the electric fields calculated without damping (Γn = 0). Within the first 50 fs of motion the electric fields emitted in the two cases are similar, but later the damping of the emitted fields for broadened levels is visible. After around 400 fs the trembling motion in real case disappears. It can be seen that the maxima of oscillations for the damped ZB motion coincide with the undamped ones. The general conclusion from Figure 9 is that the existence of disorder, many-body effects or other scattering mechanisms changes the persistent ZB motion to a decaying one, within the characteristic lifetimes for these processes: τ = 1/Γ 130 fs. Nevertheless, since the n n ≈

www.intechopen.com Zitterbewegung (Trembling Motion) Zitterbewegungof Electrons in Graphene (Trembling Motion) of Electrons in Graphene 30917 parameters Γn used in the calculations correspond to the measured lifetimes in real graphene samples, it follows that the broadening of the Landau levels does not prevent the existence of ZB. Clearly, a lower disorder in better samples will result in longer decay times for ZB. Wang et al. (2009) carried out a study similar to the one described above, but for bilayer graphene in a magnetic field. This system is somewhat different from monolayer graphene since the Landau levels are nearly uniformly spaced due to quadratic dependence of positive and negative energies on momentum, see Eq. (1). Also, the laser pulse was assumed to contain only one frequency ωL. The authors estimated that in high quality bilayer graphene samples the stimulated ZB electric field can be of the order of volts per meter and the corresponding coherence times of tens of femtoseconds.

5. Discussion and conclusions In spite of the great interest in the phenomenon of ZB its physical origin remained mysterious. As mentioned above, it was recognized that the ZB in a vacuum is due to an interference of states corresponding to positive and negative electron energies. Since the ZB in solids was treated by two-band Hamiltonians similar to the Dirac equation, its interpretation was also similar. This did not explain its origin, it only provided a way to describe it. For this reason we considered recently the fundamentals of electron propagation in a periodic potential (Zawadzki & Rusin, 2010). The physical origin of ZB is essential because it resolves the question of its observability. The second purpose was to decide whether the two-band k.p model of the band structure, used to describe the ZB in solids, was adequate. It is often stated that an electron moving in a periodic potential behaves like a free particle characterized by an effective mass m∗. The above picture suggests that, if there are no external forces, the electron moves in a crystal with a constant velocity. This, however, is clearly untrue because the electron velocity operator vˆi = pˆi/m0 does not commute with 2 the Hamiltonian Hˆ = pˆ /2m0 + V(r), so that vˆi is not a constant of the motion. In reality, as the electron moves in a periodic potential, it accelerates or slows down keeping its total energy constant. This situation is analogous to that of a roller-coaster: as it goes down losing its potential energy, its velocity (i.e. its kinetic energy) increases, and when it goes up its velocity decreases. We first considered the trembling frequency ωZ. The latter is easy to determine if we assume, in the first approximation, that the electron moves with a constant average velocity v¯ and the period of the potential is a,soωZ = 2πv¯/a. Putting typical values for GaAs: a = 5.66Å, v¯ = 2.3 107cm/s, one obtainsh ¯ ω = 1.68eV, i.e. the interband × Z frequency since the energy gap is E 1.5eV. The interband frequency is in fact typical for g ≃ the ZB in solids. One can go further calculating classical velocity oscillations for a periodic 2 potential using a condition of the energy conservation: mvz /2 + eV(z)=E, which for a periodic potential V(z) gives velocity oscillations. Finally, we used a quantum approach employing the Kronig-Penney delta-like potential since it allows one to calculate explicitly the eigenenergies and eigenfunctions (Kronig & Penney, 1931; Smith, 1961). The oscillations of the packet velocity calculated directly from the periodic potential have many similarities to those computed on the basis of the two-band k.p model. The question arises: does one deal with the same phenomenon in the two cases? To answer this question we calculated ZB using the two methods for the same periodic potential. It turned out that the two-band k.p model gives an excellent description of ZB for instantaneous velocities. This agreement demonstrates that the theories based on: (a) the periodic potential and (b) the band structure, describe the

www.intechopen.com 18310 GrapheneWill-be-set-by-IN-TECH Simulation same trembling motion of the electron. The procedure based on the energy band structure is more universal since it also includes cases which do not seem to have a direct classical interpretation. The main conclusion is that the electron Zitterbewegung in crystalline solids is the basic way of electron propagation in a periodic potential. The established nature of ZB indicates that the latter should certainly be observable. Another important conclusion is that, in spite of similarities between electron ZB in a vacuum and in crystalline solids, the origin of the phenomenon in the two situations is completely different. Recently there appeared many propositions to simulate the Dirac equation and the resulting phenomena with the use of other systems. Since in narrow-gap semiconductors and in graphene one deals with the Hamiltonians resembling the Dirac equation, one can apply simulations also to electrons in these materials. Many simulations make use of trapped atoms or ions interacting with laser light. There are two essential advantages of such methods. First, it is possible to follow the interaction of laser light with few or even single atoms or ions. Second, when simulating the Hamiltomians it is possible to modify their basic parameters in order to make the ZB frequency much lower and its amplitude much larger. In consequence, they become measurable with current experimental techniques. Simulations of important Hamiltonians are carried out with the use of Jaynes-Cummings model (Johanning et al., 2009; Lamata et al., 2007; Leibfried et al., 2003) known from quantum and atomic optics. In particular, Gerritsma et al. (2010) simulated for the first time the 1+1 Dirac equation with the resulting one-dimensional Zitterbewegung using 40Ca+ trapped ions. The results agree very well with the predictions of Zawadzki & Rusin (2010). The reason of this agreement is that the theory of Zawadzki & Rusin (2010), while concerned with semiconductors, also uses an effective Dirac equation. Gerritsma et al. (2010) showed that, if the wave packet does not have the initial momentum, the decay time of ZB is much slower. This agrees with theoretical results for carbon nanotubes, as shown in our Figure 3. An important recognition won after the considerable effort of the last years is, that the Zitterbewegung is not a marginal, obscure and probably unobservable effect, but a real and universal phenomenon that often occurs in both quantum and non-quantum systems. Clearly, the ZB in a vacuum proposed by Schroedinger (1930) stands out as an exception since it is supposed to occur without any external force. However, in its original form it is probably not directly observable for years to come and one has to recourse to its simulations. On the other hand, manifestations of ZB in crystalline solids and other periodic systems turned out to be quite common and they are certainly observable. A universal background underlying the phenomenon of ZB in any system (including a vacuum) is an interference of states belonging to positive and negative energies (in a generalized sense, see below). The positive and negative energies belong usually to bands but they can also be discrete levels, as shown for electrons in graphene in a magnetic field, see Figure 4. A question arises: what should be called “Zitterbewegung”? It seems that the signature of ZB phenomenon is its interband frequency, in which the term interband has the meaning “between interacting bands”. An instructive example is provided by graphene in a magnetic field (see Figure 4), where the electron motion contains both intraband and interband frequencies. We believe that only the interband contributions should be called ZB, while the intraband ones are simply the cyclotron components. It appears that the second signature of ZB is the actual motion which, for instance, distinguishes it from the Rabi oscillations. If an electron is prepared in the form of a wave packet, and if the electron spectrum is not completely quantized, the ZB has a transient character, i.e. it decays in time. One can

www.intechopen.com Zitterbewegung (Trembling Motion) Zitterbewegungof Electrons in Graphene (Trembling Motion) of Electrons in Graphene 31119 show that the decay time is inversely proportional to the momentum spread Δk of the wave packet, see Eq. (6). Physically, the transient character of ZB comes about as a result of waning interference of the two sub-packets belonging to positive and negative energies as they go apart because of different speeds, see Eqs. (14) and (15). The decay time is usually much longer in one-dimensional systems, see Figure 3 and Rusin & Zawadzki (2007b). On the other hand, if the electron spectrum is discrete, ZB persists in time, sometimes in the form of collapse-revival patterns. In general, the wave packet should have a non-vanishing initial momentum in one direction to exhibit the ZB in the perpendicular direction, but this is not always the case. One should ask the question about possible observation of Zitterbewegung in graphene. Two different ways were proposed to observe the trembling electrons. The first is to detect an ac current related to the ZB velocity, see Figure 2. One needs a current meter sensitive to the ZB frequency. Then, even if the electrons do not move in phase so that the net current averages to zero, the meter should detect a clear increase of noise at the frequency ωZ. The second possible way to observe the ZB is to detect electromagnetic radiation emitted by the trembling electrons, see Figure 6 and Rusin & Zawadzki (2008). The emission is possible because, if the electrons are prepared in form of wave packets or they respond to light wave packets, they are not in their eigenstates. Castro Neto et al. (2009) describing electronic properties of graphene considered possible manifestations of ZB in electron transport due to confinement of electron motion. The proposed ZB should not be confused with the Bloch oscillations of charge carriers in superlattices. The Bloch oscillations are basically a one-band phenomenon and they require an external electric field driving electrons all the way to the Brillouin zone boundary. On the other hand, the ZB needs at least two bands and it is a no-field phenomenon. Narrow gap superlattices and graphene can provide a suitable system for its observation.

6. Appendix A In this appendix we describe the time evolution of electrons in monolayer graphene in the presence of a magnetic field using operator techniques rather than averages. The initial Hamiltonian for the problem reads

Hˆ = uσxπˆ x + uσyπˆ y, (33) where πˆ = pˆ qA is the generalized momentum, q is the electron charge, σ are Pauli matrices. − i Taking the magnetic field B z we choose the vector potential A =( By,0). For an electron − there is q = e with e > 0. One can look for solutions of the Schrodinger equation in the form − Ψ(r)=eikx xΦ(y), (34) which gives an effective Hamiltonian Hˆ

Hˆ = ch¯ (k eBy/¯h)σ +(∂/i∂y)σ . (35) x − x y  Introducing the magnetic radius L = √h¯ /eB and ξ = y/L k L one has y = ξL + k L2, − x x eB/¯h = 1/L2, and ∂/∂y =(1/L)∂/∂ξ. Defining the standard raising and lowering operators for the harmonic oscillator aˆ =(ξ + ∂/∂ξ)/√2, (36) aˆ+ =(ξ ∂/∂ξ)/√2,  −

www.intechopen.com 20312 GrapheneWill-be-set-by-IN-TECH Simulation one has [aˆ, aˆ+]=1 and ξ =(aˆ + aˆ+)/√2. The rewritten Hamiltonian Hˆ is

0 aˆ Hˆ = h¯ ω , (37) − aˆ+ 0   with ω = √2c/L. The frequency ω is often used in our considerations. Now we introduce an important two-component operator Aˆ = diag(aˆ, aˆ) and its adjoint operator Aˆ + = diag(aˆ+, aˆ+). Next we define the two-component position operators

L Yˆ = Aˆ + Aˆ + , (38) √2   L Xˆ = Aˆ Aˆ + , (39) i√2 −   in analogy to the position operators yˆ and xˆ. We intend to calculate the time dependence of Aˆ and Aˆ + and then the time dependence of Yˆ and Xˆ . To find the dynamics of Aˆ one calculates the first and second time derivatives of Aˆ using the equation of motion: Aˆ dAˆ/dt =(i/¯h)[Hˆ , Aˆ]. We have t ≡ 00 Aˆ = iω (40) t 10   01 Aˆ + = iω . (41) t − 00   The second time derivatives of Aˆ and Aˆ + are calculated following the trick proposed by Schrodinger. We use two versions of this trick

2i i Aˆ =(i/¯h)[Hˆ , Aˆ ]= Hˆ Aˆ Hˆ , Aˆ , (42) tt t h¯ t − h¯ { t} 2i i Aˆ + =(i/¯h)[Hˆ , Aˆ +]= Aˆ + Hˆ + Hˆ , Aˆ + . (43) tt t − h¯ t h¯ { t } There is (i/¯h) Hˆ , Aˆ = ω2 Aˆ and (i/¯h) Hˆ , Aˆ + = ω2 Aˆ +. In consequence we obtain { t} { t } − second order equations for Aˆ and Aˆ +

Aˆ =(2i/¯h)Hˆ Aˆ ω2 Aˆ (44) tt t − Aˆ + = (2i/¯h)Aˆ + Hˆ Aˆ +ω2. (45) tt − t − To solve the above equations one eliminates the terms with the first derivative using the substitutions Aˆ = exp(+iHtˆ /¯h)Bˆ and Aˆ + = Bˆ+ exp( iHtˆ /¯h), which gives − Bˆ = (1/¯h2)Hˆ 2Bˆ ω2Bˆ, . (46) tt − − Bˆ+ = (1/¯h2)Bˆ+ Hˆ 2 Bˆ+ω2. (47) tt − −

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Finally

Bˆ = (Ωˆ 2 + ω2)Bˆ, (48) tt − Bˆ+ = Bˆ+(Ωˆ 2 + ω2), (49) tt − where Ωˆ = Hˆ /¯h. The solutions of the above equations are

iMtˆ iMtˆ Bˆ = e− Cˆ1 + e Cˆ2, (50)

ˆ+ ˆ+ iMtˆ ˆ+ iMtˆ B = C1 e− + C2 e , (51) where Mˆ =+ Ωˆ 2 + ω2 is the positive root of Mˆ 2 = Ωˆ 2 + ω2. The operator Mˆ is an ˆ ˆ+ important quantity in our considerations. Both C1 and C2 are time-independent operators. Coming back to Aˆ(t) and Aˆ +(t) one has

iΩˆ t iMtˆ iΩˆ t +iMtˆ Aˆ(t)=e e− Cˆ1 + e e C2, (52)

ˆ + ˆ+ +iMtˆ iΩˆ t ˆ+ iMtˆ iΩˆ t A (t)=C1 e e− + C2 e− e− . (53) In order to find the final forms of Aˆ(t) and Aˆ +(t) one has to use the initial conditions. They are

Aˆ(0)=Cˆ1 + Cˆ2, ˆ + ˆ+ ˆ+ A (0)=C1 + C2 , Aˆ (0)=i(Ωˆ Mˆ )Cˆ + i(Ωˆ + Mˆ )Cˆ , t − 1 2 Aˆ +(0)= iCˆ+(Ωˆ Mˆ ) iCˆ+(Ωˆ + Mˆ ). t − 1 − − 2 Simple manipulations give

i 1 1 1 1 Cˆ = Mˆ − Aˆ (0)+ Mˆ − Ωˆ Aˆ(0)+ Aˆ(0), (54) 1 2 t 2 2

i 1 1 1 1 Cˆ = Mˆ − Aˆ (0) Mˆ − Ωˆ Aˆ(0)+ Aˆ(0). (55) 2 − 2 t − 2 2 Similarly

+ i + 1 1 + 1 1 + Cˆ = Aˆ (0)Mˆ − + Aˆ (0)Ωˆ Mˆ − + Aˆ (0), (56) 1 − 2 t 2 2

+ i + 1 1 + 1 1 + Cˆ = Aˆ (0)Mˆ − Aˆ (0)Ωˆ Mˆ − + Aˆ (0). (57) 2 2 t − 2 2

One can see by inspection that the initial conditions for Aˆ(0) and Aˆ t(0) are satisfied. It is convenient to express Aˆ in terms of Aˆ and Ωˆ using the equation of motion iAˆ = AˆΩˆ Ωˆ Aˆ. t t − Then the first and second terms in Eqs. (54) and (56) partially cancel out and the operator Aˆ(t)

www.intechopen.com 22314 GrapheneWill-be-set-by-IN-TECH Simulation can be expressed as a sum Aˆ(t)=Aˆ1(t)+Aˆ2(t), where

1 iΩˆ t iMtˆ 1 Aˆ (t)= e e− Aˆ(0)+Mˆ − Aˆ(0)Ωˆ , (58) 1 2   1 iΩˆ t +iMtˆ 1 Aˆ (t)= e e Aˆ(0) Mˆ − Aˆ(0)Ωˆ . (59) 2 2 −   ˆ + ˆ + ˆ + Similarly, one can break A (t)=A1 (t)+A2 (t), where

+ 1 + + 1 +iMtˆ iΩˆ t Aˆ (t)= Aˆ (0)+Ωˆ Aˆ (0)M− e e− , (60) 1 2   + 1 + + 1 iMtˆ iΩˆ t Aˆ (t)= Aˆ (0) Ωˆ Aˆ (0)M− e− e− . (61) 2 2 −   Using Eqs. (38) and (39) we obtain

L + + Yˆ (t)= Aˆ1(t)+Aˆ2(t)+Aˆ (t)+Aˆ (t) , (62) √2 1 2   L + + Xˆ (t)= Aˆ1(t)+Aˆ2(t) Aˆ (t) Aˆ (t) . (63) i√2 − 1 − 2   The above compact equations are final expressions for the time dependence of Aˆ(t) and Aˆ +(t) operators and, by means of Eqs. (62) and (63), for the time dependence of the position operators Yˆ (t) and Xˆ (t). These exact results are given in terms of operators Ωˆ and Mˆ .To finalize this description one needs to specify the physical sense of functions of these operators appearing in Eqs. (58)-(63). As it will be seen below, operators Ωˆ and Mˆ have the same eigenfunctions, so they commute. Then the product of two exponential functions in Eqs. (58)-(61) is given by the exponential function with the sum of two exponents. In consequence, there appear two + sets of frequencies ω and ω− corresponding to the sum and the difference: ω− Mˆ Ωˆ , + ∼ − and ω Mˆ + Ωˆ , respectively. The first frequencies ω−, being of the intraband type, lead ∼ + in the non-relativistic limit to the cyclotron frequency ωc. The interband frequencies ω correspond to the Zitterbewegung. The electron motion is a sum of different frequency components. In absence of a magnetic field there are no intraband frequencies and only one interband frequency. Each of the operators Aˆ(t) or Aˆ +(t) contains both intraband and interband terms. One could infer from Eqs. (59) and (61) that the amplitudes of interband and intraband terms are similar. However, when the explicit forms of the matrix elements of Aˆ(t) and Aˆ +(t) are calculated, it turns out that the ZB terms are much smaller than the cyclotron terms, except at high magnetic fields. The operators Ωˆ and Mˆ do not commute with Aˆ or Aˆ +. In Eq. (59) the operator Aˆ acts on the exponential terms from the right-hand side, while in Eq. (61) the operator Aˆ + acts from the left-hand side. Let us consider the operator Mˆ 2 = Ωˆ 2 + ω2. Let E /¯h and n be the eigenvalue and n |  eigenvector of Ωˆ , respectively. Then

ˆ 2 ˆ 2 2 1 2 2 2 M n =(Ω + ω ) n = En + h¯ ω n . (64) |  |  h¯ 2 |   

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ˆ 2 2 Thus, every state n is also an eigenstate of the operator M with the eigenvalue λn = 2 2 2 |  En/¯h + ω . To find a more convenient form of λn we must find an explicit form of En. To do this we choose again the Landau gauge A =( By,0). Then, the eigenstate n − |  is characterized by three quantum numbers: n, kx, s, where n is the harmonic oscillator number, k is the wave vector in x direction and s = 1 labels the positive and negative x ± energy branches. The state n in a magnetic field is |  eikx x s n 1 n = − | −  , (65) |  N n n  |  

The energies of electrons in graphene are Ens = sh¯ ω√n and the norm is Nn = 4π for n > 0 and N0 = 2π. The harmonic oscillator states are

1 1/2ξ2 r n = Hn(ξ)e− , (66)  |  2π√LCn

n where Hn(ξ) are the Hermite polynomials and Cn = 2 n!√π. Using the above forms for n and E we obtain from Eq. (64) |  ns  Mˆ 2 n = ω(n + 1) n , (67) |  |  i.e. λ = ω√n + 1 = ω , where ω = ω√n. In further calculations we assume λ to n ± ± n+1 n n be positive. The operator Mˆ 2 is diagonal and its explicit form is Mˆ 2 = diag[aˆ aˆ+, aˆ+aˆ], see Eq. (64). Because Mˆ 2 = Ω2 + ω2, the eigenstates of Mˆ 2 do not depend on the energy branch index s. To calculate the functions of operators Ωˆ and Mˆ we use the fact that, for every reasonable function f of operators Ωˆ or Mˆ 2 there is f (Ωˆ )=∑ f (sω ) n n , and f (Mˆ 2)= n n |  | ∑ f (λ2 ) n n , see e.g Feynmann (1972). Thus n n |  | iΩˆ t istω e± = ∑ e± n n n , (68) n |  | 2 1/2 Mˆ =(Mˆ ) = ν ∑ λn n n , (69) n |  | 1 2 1/2 1 Mˆ − =(Mˆ )− = ν ∑ n n , (70) n λn |  | iMtˆ it(Mˆ 2)1/2 iνtλ e± = e± = ∑ e± n n n , (71) n |  | where ν = 1. Without loss of generality we take ν =+1. The above formulas can be used in ± calculating the matrix elements of Aˆ(t) and Aˆ +(t). Taking the eigenvectors n = n, kx, s and n′ = n′, k′x, s′ with n′ = n + 1, we calculate ˆ |  ˆ|  |  |  ˆ matrix elements An,n′ (t) using A(t) given in Eqs. (58) and (59). The selection rules for An,n′ (0) ˆ 1 ˆ ˆ are kx = k′x, while there are no selection rules for s, s′. The matrix element of M− A(0)Ω appearing in Eqs. (58) and (59) is

1 ˆ 1 ˆ Ωˆ ˆ ˆ n M− A(0) n′ = A(0)n,n′ s′ωn′ = s′ A(0)n,n′ . (72)  | |  λn

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√ In the last equality we used ωn′ = ωn+1 and λn = ω n + 1. Then

1 i(sω λ )t Aˆ (t) = e n − n (1 + s′)Aˆ(0) , (73) 1 n,n′ 2 n,n′ 1 i(sω +λ )t Aˆ (t) = e n n (1 s′)Aˆ(0) . (74) 2 n,n′ 2 − n,n′ ˆ ˆ ˆ Thus the matrix element of A(t)n,n′ = A1(t)n,n′ + A2(t)n,n′ is a sum of two terms, of which the first is nonzero for s =+1, while the second is nonzero for s = 1. One can show that the ′ ′ − matrix elements given in Eqs. (73) and (74) are equal to the matrix elements of the Heisenberg operator Aˆ(t) = n eiΩt Aˆ(0)e iΩt n . For Aˆ +(t) = Aˆ +(t) + Aˆ +(t) one obtains n,n′  | − | ′ n′,n 1 n′,n 2 n′,n in a similar way

+ 1 i(+λ sω )t + Aˆ (t) = e n − n (1 + s′)Aˆ (0) , (75) 1 n′,n 2 n′,n + 1 i( λ sω )t + Aˆ (t) = e − n − n (1 s′)Aˆ (0) . (76) 2 n′,n 2 − n′,n Formulas (73)-(76) describe the time evolution of the matrix elements of Aˆ(t) and Aˆ +(t) calculated between two eigenstates of Ωˆ . The frequencies appearing in the exponents are c of the form ωn+1 ωn. The intraband terms characterized by ωn = ωn+1 ωn correspond ± ± Z − to the cyclotron motion, while the interband terms characterized by ωn = ωn+1 + ωn describe ˆ ( ) ˆ ( ) ˆ +( ) ˆ +( ) ZB. Different values of s, s′ in the matrix elements of A1 t n,n′ , A2 t n′,n, A1 t n′,n, A2 t n′,n give contributions either to the cyclotron or to the ZB motion. The exact compact results given in Eqs. (73)-(76) indicate that our choice of Aˆ(t) and Aˆ +(t) operators for the description of electrons in graphene in a magnetic field was appropriate. To complete the operator considerations of ZB we calculate the matrix elements of Aˆ(t).We take n = n, k ,1 and n = n + 1, k , s . The matrix elements of Aˆ(t) for the cyclotron |  | x  | ′ | x  n,n′ and ZB components are

Aˆ(t) =(√n + 1 √n )eiω(√n √n+1 )t, (77) n,n′ ± ∓ where the upper signs correspond to the cyclotron and the lower ones to the ZB motion, ˆ + respectively. For A (t)n,n′ there is

Aˆ +(t) =(√n + 1 √n )eiω(√n+1 √n )t. (78) n,n′ ± ∓ The above results describe exact dynamics of electrons in monolayer graphene in the presence of an external magnetic field. This description is equivalent to the one given in the text but it is more general since it is not related to a specific electron wave packet.

7. Appendix B We briefly discuss here the classical electron velocity and mass for a linear energy band of monolayer graphene, as they are often subjects of misunderstandings. Let us consider the conduction band and take p 0, where the pseudo-momentum is p = h¯ k. Then the band ≥

www.intechopen.com Zitterbewegung (Trembling Motion) Zitterbewegungof Electrons in Graphene (Trembling Motion) of Electrons in Graphene 31725 dispersion is E = up and the classical velocity is

∂E dE ∂p dE pi dE 1 vi = = = = δijpj, (79) ∂pi dp ∂pi dp p dp p where δij is the Kronecker delta function and we use the sum convention over the repeated index j = 1, 2. The electron mass tensor mˆ relating the velocity to pseudo-momentum is defined by mˆ v = p. Then the inverse mass tensor (1/ˆm) is defined by

1 v = p . (80) i m j  ij Equating Eq. (79) with Eq. (80) we obtain

1 dE 1 = δ . (81) m dp p ij  ij Thus the inverse mass tensor is a scalar: 1/m =(dE/dp)(1/p). Using the initial band dispersion one has dE/dp = u, so that m = p/u = E/u2. This equality can be seen in two ways. First, it gives E = mu2, (82) which is analogous to the Einstein relation between the particle energy and mass. Second, the formula E m = (83) u2 states that the mass vanishes at E = 0 (or p = 0), but is nonzero for E > 0 (or p > 0). These relations hold also for a more general “semi-relativistic” case of narrow-gap semiconductors, see Zawadzki (1997; 2006). If a force F is applied to the electron, the relation

dp = F (84) dt is always valid. In our case the pseudo-momentum p = mu, where u is the constant velocity. Thus the force does not accelerate the electron, it only changes its mass. One should add that, if one defined the mass by the relation of the force to acceleration: Mˆ a = F , the inverse mass would be given by the second derivative of the energy with respect to pseudo-momentum. For the linear band of graphene: E = up, the second derivative of E vanishes, so that such a mass would be infinitely large for all energies. Thus, it is not a useful quantity.

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Maksimova, G. M, Demikhovskii, V Y & Frolova, E V (2008). Wave packet dynamics in a monolayer graphene. Phys. Rev. B Vol. 78, No. 23, 15 December 2008, 235321 [7 pages] (arXiv:0809.0367) Martinez, J. C.; Jalil, M. B. A. & Tan, S. G. (2010). Klein tunneling and zitterbewegung and the formation of a polarized p-n junction in graphene. Appl. Phys. Lett. Vol. 97, No. 6, 9 Aug 2010, 062111 [3 pages](arXiv:0806.0222) McCann, E. & Fal’ko V. I. (2006). Landau-Level Degeneracy and Quantum Hall Effect in a Graphite Bilayer. Phys. Rev. Lett. Vol. 96, No. 8, 3 March 2006, 086805 [4 pages] (arXiv:0510237) Novoselov, K. S.; Geim.; A. K.; Morozov, S. V.; Jiang, D.; Zhang, Y.; Dubonos, S. V.; Grigorieva, I. V. & Firsov, A. A. (2004). Electric Field Effect in Atomically Thin Carbon Films. Science Vol. 306, No. 5696, 22 October 2004, 666–669 (arXiv:0410631) Romera, E. & de los Santos, F. (2009). Revivals, classical periodicity, and zitterbewegung of electron currents in monolayer graphene. Phys. Rev. B Vol. 80, No. 16, 15 October 2009, 165416 [5 pages] (arXiv:0911.4367) Rusin, T. M. & Zawadzki, W. (2007a). Zitterbewegung of nearly-free and tightly-bound electrons in semiconductors. J. Phys. Cond. Matter Vol. 19, No. 13, 4 April 2007, 136219 [18 pages] (arXiv:0605384) Rusin, T. M. & Zawadzki, W. (2007b). Transient Zitterbewegung of charge carriers in mono- and bilayer graphene, and carbon nanotubes. Phys. Rev. B Vol. 76, No. 19, 15 November 2007, 195439 [7 pages] (arXiv:0702425) Rusin, T. M. & Zawadzki, W. (2008). Zitterbewegung of electrons in graphene in a magnetic field. Phys. Rev. B Vol. 78, No. 12, 15 September 2008, 125419 [9 pages] (arXiv:0712.3590) Rusin, T. M. & Zawadzki, W. (2009). Theory of electron Zitterbewegung in graphene probed by femtosecond laser pulses. Phys. Rev. B Vol. 80, No. 4, 15 July 2009, 045416 [9 pages] (arXiv:0812.4773) Sakurai, J. J. (1987). Modern Quantum Mechanics, Addison-Wesley, ISBN 9780201539295, New York Schliemann, J.; Loss, D. & Westervelt, R. M. (2005). Zitterbewegung of Electronic Wave Packets in III-V Zinc-Blende Semiconductor Quantum Wells. Phys. Rev. Lett. Vol. 94, No. 20, 27 May 2005, 206801 [4 pages] (arXiv:0410321) Schliemann, J. (2008). Cyclotron motion in graphene. New J. Phys. Vol. 10, April 2008, 034024 [9 pages] (arXiv:0802.1396) Schrodinger, E. (1930). Ueber die kraeftefreie Bewegung in der relativistischen Quantenmechanik. Sitzungsber. Preuss. Akad. Wiss. Phys. Math. Kl. 24, 418–428. Schrodinger’s derivation is reproduced in Barut & Bracken (1981) Semenoff, G. W. (1984). Condensed-Matter Simulation of a Three-Dimensional Anomaly. Phys. Rev. Lett. Vol. 53, No. 26, 24 December 1984, 2449–2452 Slonczewski, J. C. & Weiss, P. R. (1958). Band Structure of Graphite. Phys. Rev. Vol. 109, No. 2, January 1958, 272–279 Smith, R. A. (1961). Wave Mechanics of Crystalline Solids, Chapman & Hall, ISBN 0412093707, London Vonsovskii, S. V.; Svirskii, M. S. & Svirskaya, L. M. (1990). Zitterbewegung of a band electron. Teor. Matem. Fizika Vol. 85, No. 2, November, 1990, 211–221; Theor. and Math. Physics, Vol. 85, No. 2, 1159–1167

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ISBN 978-953-307-556-3 Hard cover, 376 pages Publisher InTech Published online 01, August, 2011 Published in print edition August, 2011

Graphene, a conceptually new class of materials in condensed-matter physics, has been the interest of many theoretical studies due to the extraordinary thermal, mechanical and electrical properties for a long time. This book is a collection of the recent theoretical work on graphene from many experts, and will help readers to have a thorough and deep understanding in this fast developing field.

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